Evolution of clouds on Titan over 30 hours between November 4 and November 6, 2022, as seen by Webb NIRCam (left) and Keck NIRC-2 (right). Titan’s trailing hemisphere seen here is rotating from left (dawn) to right (evening) as seen from Earth and the Sun. Cloud A appears to be rotating into view while Cloud B appears to be either dissipating or moving behind Titan’s limb (around toward the hemisphere facing away from us). Clouds are not long-lasting on Titan or Earth, so those seen on Nov. 4 may not be the same as those seen on Nov. 6. The NIRCam image used the following filters: Blue=F140M (1.40 microns), Green=F150W (1.50 microns), Red=F200W (1.99 microns), Brightness=F210M (2.09 microns). The Keck NIRC-2 image used: Red=He1b (2.06 microns), Green=Kp (2.12 microns), Blue=H2 1-0 (2.13 microns).
Credits
Science
NASA, ESA, CSA, Webb Titan GTO Team
Image Processing
Alyssa Pagan (STScI)
About The Object | |
---|---|
Object Name | Titan |
Object Description | Saturn's moon |
About The Data | |
Data Description | This image was created with Webb data from proposal (C. Nixon) |
Instrument | Webb> NIRCam Keck> NIRC-2 |
Exposure Dates | 4 Nov 2022, 6 Nov 2022 |
Filters | Left: F140M, F150W, F200W, F210M Right: He 1b, Kp, H2 1-0 |
About The Image | |
Color Info | These images are a composite of separate exposures acquired by the James Webb Space Telescope using the NIRCam instrument and the Keck Telescope using the NIRC-2 instrument. Several filters were used to sample different infrared wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Left> Blue: F140M (1.4 microns), Green: F150W (1.5 microns), Red: F200W (2.0 microns), Luminosity: F210M (2.1 microns) Right> Red: He1b (2.06 microns), Green: Kp (2.12 microns), Blue: H2 1-0 (2.13 microns) |
About The Object | |
---|---|
Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
Object Description | The type of astronomical object. |
R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
About The Data | |
Data Description |
|
Instrument | The science instrument used to produce the data. |
Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
Filters | The camera filters that were used in the science observations. |
About The Image | |
Image Credit | The primary individuals and institutions responsible for the content. |
Publication Date | The date and time the release content became public. |
Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |